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Table 1.

Summary of the simulations.

Run Prot [days] urms [m/s] Brms [kG] Co Ta[108] Pe Re ReM RiΩ[10−2] Pcyc [years]
MHDr1 20 99 no dynamo 5.0 1.10 11 52 36 16.0
MHDr2 15 51 60 10.1 1.95 7 35 24 9.2 1.81 ± 0.10
MHDr2* 15 52 57 9.9 1.95 7 35 25 9.2 2.14 ± 0.13
MHDr3 10 39 65 19.2 4.38 5 27 19 4.1 2.50 ± 0.11
MHDr3* 10 39 62 18.8 4.38 5 28 19 3.9 2.62 ± 0.14
MHDr4 8 35 60 26.9 6.84 5 24 17 2.6 3.14 ± 0.05
MHDr4* 8 35 57 26.2 6.84 5 25 17 2.5 3.37 ± 0.08

zMHDr1 20 95 not saturated 4.9 1.10 11 53 37 16.8
zMHDr2 15 55 49 9.6 1.95 7 36 25 9.6 1.95 ± 0.03
zMHDr3 10 39 53 18.9 4.38 5 28 19 4.3 2.60 ± 0.03
zMHDr4 8 36 46 26.9 6.84 5 24 17 2.7 2.50 ± 0.02

Notes. From left to right, the columns correspond to: the rotation period Prot = 2π0, the volume averaged (over the convective zone) rms flow velocity urms, the volume-averaged rms magnetic field Brms, the Coriolis number, the Taylor number, the SGS Péclet number, the fluid and magnetic Reynolds numbers, the Richardson number averaged over the radiative zone, and the magnetic cycle period.

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